Aurel Ironbark OIII nebula filter 1.25 in, observatory grade
OIII · 1.25 in · 8 nm bandpass
$99
Catalog preview. Not available for purchase.
- Grade
- Observatory grade
- Coating
- Anti-reflection on both faces
- Case
- Plastic case
- Edition
- 2026 edition
Specifications
| Filter type | OIII nebula filter |
|---|---|
| Cell | 1.25 in brass cell, M28.5 x 0.6 thread |
| Bandpass (FWHM) | 8 nm |
| Peak transmission | 90% |
| Substrate | Optical glass |
| Glass thickness | 1.5 mm |
| Grade | Observatory grade |
| Coating | Anti-reflection on both faces |
| Case | Plastic case |
| Edition | 2026 edition |
Description
The Ironbark OIII is a narrowband nebula filter in a 1.25 in threaded cell. It passes a band about 8 nm wide centered near 500 nm, which covers the doubly ionized oxygen emission lines at 496 nm and 501 nm, and it blocks most other visible wavelengths. Peak transmission is about 90 percent within that band, so the oxygen light that reaches the eyepiece remains bright. The filter screws into the barrel of a 1.25 in eyepiece or the nosepiece of a 1.25 in diagonal. One surface carries the multi-layer interference stack and the other carries an anti-reflection layer.
Emission nebulae shine at specific wavelengths, while the sky background glows across the spectrum. By passing the oxygen lines and blocking the rest, the filter lowers the background brightness around a nebula, so faint outer structure stands out against a darker field. The nebula itself does not gain brightness. Under moderately dark skies, you may see the Veil Nebula, the Dumbbell Nebula, and the Owl Nebula with greater detail, since their emission is strong in the oxygen lines. Oxygen-rich planetary nebulae and supernova remnants respond best to this filter.
The filter does not help with galaxies, star clusters, or reflection nebulae, which emit across a broad range of wavelengths, so on those targets it mainly dims the view. Hydrogen-emission nebulae such as the Orion Nebula contain comparatively little oxygen emission, so a UHC or H-beta filter is usually the better choice for them. Because much of the light is removed, the filter works best in telescopes of 150 mm aperture or larger, under dark skies, at low magnification that frames the target without spreading its light too thinly. Allow your eyes about twenty minutes to dark-adapt before observing, and keep the cell capped when the filter is not in use. Stars appear strongly dimmed through this filter, so star fields look sparse.
About this configuration
The Aurel Ironbark OIII nebula filter 1.25 in is offered in several configurations, and the notes below describe what this particular one includes. The observatory grade comes with a measured transmission curve for the individual filter in the box. Observatory grade glass has the tightest flatness tolerance in the Ironbark line, which suits imaging with long focal lengths. With anti-reflection layers on both sides, less light bounces between the filter and the eyepiece or camera sensor.
The filter ships in a clear plastic case that keeps dust off the glass between sessions. This is the 2026 edition, the most recent version of the Ironbark line in the catalog. A filter does not make objects brighter; it darkens the sky background more than the target, which raises contrast.
What's in the box
- OIII filter in 1.25 in threaded cell
- Plastic storage case
- Test report with measured transmission curve
- Plastic storage case
Compatibility notes
- Threads into 1.25 in eyepieces, diagonals, and filter wheels (M28.5 x 0.6).
- Most effective in telescopes of 150 mm aperture and larger under dark skies.